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Journal ArticleDOI

Ca-, Al-Rich Inclusions in Two New Carbonaceous Chondrites from Grove Mountains, Antarctica

TLDR
In this paper, a survey of Ca-, Al-rich inclusions in GRV 023155 (CV3) and GRV 050179 (CM2) suggests that Type A and spinel-pyroxene inclusions are common in these two meteorites.
Abstract
Two new carbonaceous chondrites, GRV 023155 and GRV 050179, collected from the Grove Mountains (GRV), Antarctica, have been classified as the oxidized CV3 and CM2 chondrites, respectively.  A total of 9 Ca-, Al-rich inclusions (CAIs) were found in the two meteorites. Most of the inclusions are extensively altered, with phyllosilicates commonly found in the alteration assemblages of CAIs, chondrules and matrix in the GRV 050179 CM2 chondrites, suggesting that aqueous alteration occurred on the host meteorite parent body. In contrast, feldspathoids and hedenbergite were identified in the CAIs from GRV 023155. The FeO-rich phases in the CAIs from GRV 023155 indicate alteration of these CAIs happened under high oxygen fugacity. All 9 inclusions can be classified as Type A or spinel-pyroxene rich inclusions, and they probably represent a continuum of solar nebular condensation. The survey of Ca-, Al-rich inclusions in GRV 023155 (CV3) and 050179 (CM2) suggests that Type A and spinel-pyroxene inclusions are common in these two meteorites.

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Citations
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Progress of Antarctic meteorite survey and research in China

TL;DR: Miao et al. as discussed by the authors summarized the progress of Chinese meteorite survey efforts in the Grove Mountains, as well as discuss progress of the classification and investigation of Grove Mountains meteorites.
Journal ArticleDOI

A Review of Research on Grove Mountains CM-Type Chondrites

TL;DR: In this article , the authors reviewed the study of GRV CM chondrites and found that GRV 020025 is the most heavily altered chondrite with a modal content of 1.0 vol% for CAIs and amoeboid olivine aggregates.
References
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Journal ArticleDOI

A chemical-petrologic classification for the chondritic meteorites.

TL;DR: In this article, a two-dimensional classification grid based on chemical and petrologic subdivisions of chondritic meteorites is proposed, which extends the current chemical subdivisions to account for varying petrolic (implied metamorphic) properties within the primary chemical groups.
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Condensation in the primitive solar nebula

TL;DR: In this article, the distribution of the major elements between vapor and solid has been calculated for a cooling gas of cosmic composition, assuming that high temperature condensates remain in equilibrium with the vapor, affecting the temperatures of appearance of successively less refractory phases.
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The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk

TL;DR: U-corrected Pb-Pb dating from primitive meteorites indicates that chondrule formation started contemporaneously with CAIs and lasted ~3 million years, suggesting that the formation ofCAIs and chondrules reflects a process intrinsically linked to the secular evolution of accretionary disks.
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X-rays and Fluctuating X-Winds from Protostars

TL;DR: In this article, it was shown that protostars emit more x-rays, hard and soft, than young sunlike stars in more advanced stages of formation, due to the time-dependent interaction of an accretion disk with the magnetosphere of the central star.
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The Origin of Chondrules and Refractory Inclusions in Chondritic Meteorites

TL;DR: In this paper, the authors adopt the model of a fluctuating X-wind, where the inner edge of the solar nebula undergoes periodic radial excursions on a timescale of ~30 yr, perhaps in response to protosolar magnetic cycles.
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